Rarefaction of the Very Slow (<350 km/s) Solar Wind in Cycle 24 Compared With Cycle 23
Author:
Affiliation:
1. Institute for Space-Earth Environmental Research; Nagoya University; Nagoya Japan
2. Department of Natural Science and Mathematics; Chubu University; Kasugai Japan
Funder
Grant-in-Aid for Scientific Research (A)
Publisher
Wiley
Subject
Space and Planetary Science,Geophysics
Reference42 articles.
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4. Acceleration of the solar wind as a result of the reconnection of open magnetic flux with coronal loops;Fisk;Journal of Geophysical Research,2003
5. How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation;Fujiki;Annales de Geophysique,2003
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